Galaxy formation and evolution

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The Chandra Fornax survey.: I.: The cluster environment

ASTROPHYSICAL JOURNAL 633:1 (2005) 154-164

Authors:

CA Scharf, DR Zurek, M Bureau
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The SCUBA half-degree extragalactic survey -: I.: Survey motivation, design and data processing

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 363:2 (2005) 563-580

Authors:

AMJ Mortier, S Serjeant, JS Dunlop, SE Scott, P Ade, D Alexander, O Almaini, I Aretxaga, C Baugh, AJ Benson, PN Best, A Blain, J Bock, C Borys, A Bressan, C Carilli, EL Chapin, S Chapman, DL Clements, K Coppin, M Crawford, M Devlin, S Dicker, L Dunne, SA Eales, AC Edge, D Farrah, M Fox, C Frenk, E Gaztañaga, WK Gear, E Gonzales-Solares, GL Granato, TR Greve, JA Grimes, J Gundersen, M Halpern, P Hargrave, DH Hughes, RJ Ivison, MJ Jarvis, T Jenness, R Jimenez, E van Kampen, A King, C Lacey, A Lawrence, K Lepage, RG Mann, G Marsden, P Mauskopf, B Netterfield, S Oliver, L Olmi, MJ Page, JA Peacock, CP Pearson, WJ Percival, A Pope, RS Priddey, S Rawlings, N Roche, MR Robinson, D Scott, K Sekiguchi, M Seigar, L Silva, C Simpson, I Smail, JA Stevens, T Takagi, G Tucker, C Vlahakis, I Waddington, J Wagg, M Watson, C Willott, M Vaccari
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Towards simulating star formation in the interstellar medium

Monthly Notices of the Royal Astronomical Society 356 (2005) 737-752

Authors:

AD Slyz, Julien Devriendt, Greg Bryan, Joseph Silk
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NIR Spectroscopy of Luminous Infrared Galaxies and the Hydrogen Recombination Photon Deficit

(2004)

Authors:

JR Valdes, S Berta, A Bressan, A Franceschini, D Rigopoulou, G Rodighiero
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CIRPASS: Description, performance and astronomical results

Proceedings of SPIE - The International Society for Optical Engineering 5492:PART 2 (2004) 1135-1144

Authors:

I Parry, A Bunker, A Dean, M Doherty, A Horton, D King, M Lemoine-Busserole, C Mackay, R McMahon, S Medlen, R Sharp, J Smith

Abstract:

The Cambridge Infra-red Panoramic Survey Spectrograph (CIRPASS) is described. This near-infrared (MR) spectrograph has been used on the 8m Gemini-South Telescope, the 3.9m Anglo-Australian Telescope (AAT) and the 4.2m William Herschel Telescope (WHT). Its performance in both integral field mode and multi-object mode is discussed and some scientific highlights are presented. A multi-IFU system, which is currently under construction, is also described.
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